In Table REF  we present results for primary and secondary images in EQG when the source is closer to Sgr A*. In particular, we have taken \({\cal D}=0.05\) . Comparing these results those in Table REF  (in which \({\cal D}=0.5\) ), shows that when the source-lens distance is smaller, primary and secondary images get closer to the line of sight to the lens (\(\theta _{p}\)  and \(|\theta _{s}|\)  get smaller). Furthermore, a comparison of Tables REF  and REF  shows that the magnification \(\mu _{p}\)  and \(|\mu _{s}|\)  and the time delay of the primary image are smaller in the case of \({\cal D}=0.05\)  compared to \({\cal D}=0.5\) . However the differential time delay \(t_d=\tau _s-\tau _p\)  is larger in the former case. Similar results hold when the governing theory of gravity is GR [1]}.
